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Exploring Thermodynamic Properties of Earth’s Core-Forming Materials

Descrizione del progetto

I materiali che formano il nucleo della Terra: relazioni di fase e densità nei sistemi ferro-elementi leggeri

Il nucleo della Terra genera il campo magnetico terrestre. Le caratteristiche costituite al momento della sua formazione contengono informazioni sull’origine e sull’evoluzione del pianeta. Il progetto Earth core, finanziato dal Consiglio europeo della ricerca, costruirà un modello termodinamico del nucleo terrestre ricco di ferro (Fe), con particolare attenzione agli elementi leggeri e alla loro modulazione in base a pressione (P), temperatura (T) e ambiente chimico. La squadra di scienziati condurrà esperimenti ad alta P-T con vari tipi di riscaldamento, diffrazione di raggi X in situ e analisi chimiche. I risultati ispireranno dei calcoli termodinamici per ottenere proprietà fisiche difficili da determinare direttamente per via sperimentale. Gli esiti del progetto faranno luce sull’origine e sull’evoluzione della Terra e di altri pianeti terrestri con nucleo metallico.

Obiettivo

It is known that the Earth’s core is less dense than pure iron by about 7%, which is due to the presence of a light element(s) such as Si, S, C, O, and H. The goal of this project is to construct a thermodynamic model of the Earth’s central core. A particular focus is on the identification of the light element because the inclusion of these elements in iron liquid depends on the pressure (P), temperature (T), and chemical environment and hence provides us invaluable information about the origin and evolution of the solid Earth. We will examine phase relations and density of phases in Fe-light element systems by conducting high-P-T experiments and employing thermodynamic calculations based on the experimental data.
High-P-T experiments will be conducted in a diamond anvil cell with three different kinds of heating techniques: laser heating, external-resistive heating, and internal-resistive heating. Of the three, the internal-resistive heating system is a special technique that I have developed and employed and I am currently generating 5000 K at 200 GPa with it. Structure of phases will be analysed by in-situ X-ray diffraction. Chemical analysis will also be employed on samples to determine element partitioning between the phases.
I will also employ thermodynamic calculations based on the experimental data to fully understand the thermodynamic properties of the materials and obtain physical properties which are difficult to directly determine by experiment such as sound velocity of liquids.
From the thermodynamic models, I will calculate the physical properties of light element-bearing iron liquids and compare them with seismologically constrained values of the Earth’s core to find out the best matching composition. From these results, I will discuss the physical and chemical environments during the core formation and implicate in the origin and evolution of the Earth. Also the results will be applied to other terrestrial planets which have metallic cores.

Meccanismo di finanziamento

ERC-COG - Consolidator Grant

Istituzione ospitante

THE UNIVERSITY OF EDINBURGH
Contribution nette de l'UE
€ 1 891 765,00
Indirizzo
OLD COLLEGE, SOUTH BRIDGE
EH8 9YL Edinburgh
Regno Unito

Mostra sulla mappa

Regione
Scotland Eastern Scotland Edinburgh
Tipo di attività
Higher or Secondary Education Establishments
Collegamenti
Costo totale
€ 1 891 765,00

Beneficiari (1)